Astronomy and Astrophysics, volume 331, 193-210 (1998/3-1)
X-rays and star formation: ROSAT observations of the Monoceros and Rosette molecular clouds.
GREGORIO-HETEM J., MONTMERLE T., CASANOVA S. and FEIGELSON E.D.
Abstract (from CDS):
We report ROSAT observations of two molecular clouds previously unstudied in the X-ray band, examining the possibility that X-rays can serve as tracers of star formation at distances >1kpc. The targets are the molecular clouds associated with the Monoceros R2 reflection nebula (d=0.8kpc) and with the Rosette giant HII region (d=1.5kpc). In both cases, the PSPC images show point sources and extended emission. Most of the 41 distinct ROSAT sources in the Monoceros cloud and 21 sources in the Rosette cloud have optical counterparts on digitized plates, but a significant minority (20 - 30%) do not and are probably embedded in the clouds. Comparison with recent near-infrared surveys of the Monoceros and Rosette clouds supports the broad correspondence, previously found in nearby clouds, between X-ray and near-infrared sources associated with Young Stellar Objects. X-ray luminosities are LX∼1030-1032erg/s. The X-ray hardness ratios and LX/Lbol ratios of the Monoceros and Rosette X-ray sources are comparable to those found for low- and intermediate-mass pre-main sequence stars in nearby star forming clouds. We conclude that most of the point-like ROSAT sources are T Tauri and Herbig Ae/Be stars. Extended X-ray ``hot spots'' are seen in both clouds, which likely result from the partially resolved emission of embedded young star clusters, similar to the ρ Oph cluster. The detection of individual stars in the high-luminosity tail of the low-mass stellar population, and of embedded young star clusters in star-forming molecular cores, confirm that X-rays can efficiently trace low- and intermediate-mass star formation at significant distances across the Galaxy.
stars: ISM: Monoceros clouds - Rosette nebula - pre-main sequence - formation - X-rays: stars
Table 2a, 2b: [GMC98] Mon X-NN (Nos 1-48). Table 3a, 3b: [GMC98] Rosette X-NN (Nos 1-29). Table 6: [GMC98] Rosette IR-N (Nos 1-7).
Table 5: IRNNN = [CMD97] NNN
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